Rydberg Formula Calculator
Wavelengths of hydrogen spectral lines from the Rydberg formula — pick a series or two levels, get wavelength, wavenumber, frequency and photon energy, plus the series limit.
How it works
1/λ = R_∞ · Z² · (1/n₁² − 1/n₂²), R_∞ = 1.0973731 × 10⁷ m⁻¹; series limit: 1/λ = R·Z²/n₁²
Rydberg found in 1888 that every hydrogen line fits one formula with two integers — an empirical pattern Bohr explained 25 years later. Each series shares a lower level: Lyman lines end on n = 1 and lie in the UV, Balmer on n = 2 and span the visible (the four lines you see in a discharge tube), Paschen and beyond are infrared. As n₂ grows the lines crowd toward the series limit, which corresponds to ionising the atom from that level.
Worked example
Balmer n = 4 → 2: 1/λ = 1.097 × 10⁷ × (1/4 − 1/16) = 2.057 × 10⁶ m⁻¹ → λ = 486.1 nm, the blue-green H-β line.
Frequently asked questions
Why is the measured H-α 656.28 nm, not 656.11?
The infinite-mass Rydberg constant ignores nuclear recoil; using R_H = 1.09678 × 10⁷ m⁻¹ (and air vs vacuum) closes the gap.
Does it work for helium?
For He⁺ (one electron) with Z = 2, yes; neutral helium has two electrons and no simple formula.
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This calculator is for educational purposes. Double-check important results before acting on them.